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Explanation: In the Summer of 1054 A.D. Chinese astronomers reported that a star in the constellation of Taurus suddenly became as bright as the full Moon. Fading slowly, it remained visible for over a year. It is now understood that a spectacular supernova explosion - the detonation of a massive star whose remains are now visible as the Crab Nebula- was responsible for the apparition. The core of the star collapsed to form a rotating neutron star or pulsar, one of the most exotic objects known to modern astronomers. Like a cosmic lighthouse, the rotating Crab pulsar generates beams of radio, visible, x-ray and gamma-ray energy which, as the name suggests, produce pulses as they sweep across our view. Using a stunning series of visible light images taken with the Hubble Space Telescope (HST) in 1995, astronomers have discovered spectacular pulsar powered motions within the Crab nebula. Highlights of this HST Crab "movie" show wisps of material moving away from the pulsar at half the speed of light, a scintillating halo, and an intense knot of emission dancing, sprite-like, above the pulsar's pole. Only 10 kilometers wide but more massive than the sun, the pulsar's energy drives the dynamics and emission of the nebula itself which is more than 10 light-years across.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: neutron star - pulsar - Crab Nebula - supernova
Publications with words: neutron star - pulsar - Crab Nebula - supernova
See also:
- APOD: 2025 September 3 Á Cir X1: Jets in the Africa Nebula
- APOD: 2025 August 24 Á The Spinning Pulsar of the Crab Nebula
- APOD: 2025 August 8 Á Dawn of the Crab
- APOD: 2025 July 31 Á Supernova 2025rbs in NGC 7331
- M1: The Incredible Expanding Crab
- Supernova Remnant CTA 1
- APOD: 2024 July 23 Á The Crab Nebula from Visible to X Ray